2003MNRAS.341.1268P


Query : 2003MNRAS.341.1268P

2003MNRAS.341.1268P - Mon. Not. R. Astron. Soc., 341, 1268-1271 (2003/June-1)

X-ray absorption via Kα resonance complexes in oxygen ions.

PRADHAN A.K., CHEN G.X., DELAHAYE F., NAHAR S.N. and OELGOETZ J.

Abstract (from CDS):

The Kα resonance complexes in oxygen ions Oi-Ovi are theoretically computed, and resonance oscillator strengths and wavelengths are presented. The highly resolved photoionization cross-sections, with relativistic fine structure, are computed in the coupled channel approximation using the Breit-Pauli R-matrix method. A number of strong Kα resonances are found to be appreciable, with resonance oscillator strengths fr> 0.1. The Kα resonance wavelengths of Oi-Ovi lie in the relatively narrow wavelength range 22-23.5 Å, and the X-ray opacity in this region should therefore be significantly affected by K ⟶ L transitions in oxygen. The results should be useful in the interpretation of soft X-ray spectra observed from Chandra and XMM-Newton.

Abstract Copyright: 2003 RAS

Journal keyword(s): atomic data - atomic processes - line: profiles - galaxies: Seyfert - X-rays: galaxies

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 3783 Sy1 11 39 01.7096819040 -37 44 19.009642992   12.46 13.43 11.33 12.1 ~ 1765 1
2 NGC 4253 Sy1 12 18 26.5163572920 +29 48 46.531535472   14.34 13.57     ~ 1106 1
3 MCG-06-30-015 Sy1 13 35 53.7691256160 -34 17 44.160716796   13.89 13.61 8.9   ~ 1559 0

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